{"total":14,"items":[{"citing_arxiv_id":"2606.28257","ref_index":82,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"When Jets Don't Quench: Near-Infrared H$_{2}$ in Star Forming Low-Excitation Radio Galaxies","primary_cat":"astro-ph.GA","submitted_at":"2026-06-26T16:41:55+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"New Gemini/GNIRS observations of star-forming radio galaxies show warm H2 emission driven primarily by mergers rather than jets.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.06802","ref_index":44,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Radiation Pressure Instability in the \"turn-on\" Changing-Look AGN SDSS J1430+2303","primary_cat":"astro-ph.GA","submitted_at":"2026-06-05T01:03:37+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Multi-wavelength data from SDSS J1430+2303 are interpreted as evidence that radiation pressure instabilities drive a shrinking unstable accretion-disk zone, based on timing analysis, weak soft excess, and SED-derived black-hole parameters.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.01570","ref_index":30,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Morphology of Optical Changing-Look AGN-host Galaxies: Evidence for an Important Role of Mergers","primary_cat":"astro-ph.GA","submitted_at":"2026-06-01T02:18:38+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"CL-AGN host galaxies exhibit a 29% merger fraction (about 2x higher than non-CL-AGN controls) with morphology indicating modest disturbances, based on non-parametric metrics and visual inspection of DESI images.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.24429","ref_index":42,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Changing-look Active Galactic Nuclei from SDSS, LAMOST and DESI Survey","primary_cat":"astro-ph.GA","submitted_at":"2026-05-23T06:52:38+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Multi-epoch spectroscopic cross-matching yields 45 CLAGNs (43 turn-off, 2 turn-on) including 12 repeating sources that trace a high-low-high accretion-state path in the black-hole mass versus Eddington-ratio plane.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.07965","ref_index":86,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A Changing-Look Seyfert Discovered by eROSITA Reveals a Two-Component Broad-Line Region","primary_cat":"astro-ph.GA","submitted_at":"2026-05-08T16:28:42+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"HE 1237-2252 exhibits a changing-look event driven by intrinsic accretion-rate variations, revealing a two-component broad-line region consisting of virialized gas at ~27 light-days and disk emission at larger radii.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.05298","ref_index":285,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Kinematic Stratification in Extremely Red Quasars Revealed by JWST","primary_cat":"astro-ph.GA","submitted_at":"2026-05-06T18:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"JWST observations of ERQs show stratified gas kinematics via deblended optical emission lines, with UV lines dominated by scattered light and optical lines mixing scattered and obscured emission.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.03577","ref_index":24,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Optical Variability Structure Function of Low-Luminosity AGN using ATLAS Lightcurves","primary_cat":"astro-ph.GA","submitted_at":"2026-05-05T09:45:16+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Low-luminosity AGN exhibit structure function slopes rising from 0.1 to 0.3 with black hole mass, no breaks on decadal scales, amplitude anticorrelated with luminosity and positively correlated with mass.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.21390","ref_index":4,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A Synchronized Spin Model for Black-Hole Accretion Systems","primary_cat":"astro-ph.HE","submitted_at":"2026-04-23T07:58:43+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"A model of accretion-disk dynamos as synchronized macro-spins unifies broadband variability, coronal heating, jets, and hard/soft cycles via collective spin dynamics.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"wind and P disc wind denote continuous and discrete wind power, respectively. (vi) State transitions and excursions. In XRBs, hardness, timing properties, jet behavior, and bro ad outflow signatures reorganize together along the HID/q-diagram [2]. In AGN, changing-loo k events indicate that large spectral changes need not be accompanied by equally strong new jets [4 , 5]. Any successful model must therefore distinguish full large-scale magnetic reorgani zation from more limited excursions in magnetic state space. These constraints motivate a nonequilibrium magnetic desc ription in which timing statistics and outflow morphology arise from the same evolving collecti ve variables. 5 3 Physical Basis of the Synchronized Spin Model (SSM)"},{"citing_arxiv_id":"2604.19435","ref_index":88,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"SDSSJ110546.07+145202.4: The first long-duration radio changing-look NLS1 galaxy","primary_cat":"astro-ph.HE","submitted_at":"2026-04-21T13:09:40+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"SDSSJ110546.07+145202.4 is the first known long-duration radio changing-look NLS1 galaxy whose outburst is explained by an accretion-rate change that triggered a powerful radio jet.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.12109","ref_index":71,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Identifying Changing-Look AGN Transitions in Light Curve Data with the Zwicky Transient Facility","primary_cat":"astro-ph.GA","submitted_at":"2026-04-13T22:32:22+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A criterion of |Δg| > 0.4 mag and |Δ(g-r)| > 0.2 mag detects photometric CL-AGN transitions in 9.6% of known hosts with 1.6% false positive rate from simulations.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.07561","ref_index":45,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Tracing Active Galactic Nuclei Properties Through a Changing-look Event","primary_cat":"astro-ph.GA","submitted_at":"2026-04-08T20:02:30+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"A changing-look AGN exhibits a rapid accretion-driven spectral transition with broad-line region temperatures of approximately 11,800 K measured via Boltzmann plots and stable black hole mass estimates of 5 times 10 to the 7 solar masses across epochs.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2512.02836","ref_index":41,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The Large Sky Area Multi-object Fiber Spectroscopic Telescope (LAMOST) Quasar Survey: Quasar Properties from Data Release 10 to 12","primary_cat":"astro-ph.GA","submitted_at":"2025-12-02T14:44:32+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"LAMOST DR10-12 adds 11,346 quasars (5,386 new) with ZTF-recalibrated spectra and derived emission-line and black-hole mass properties to support variability and rare-object studies.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2511.09626","ref_index":18,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Changing-Look AGN Powered By Disk Tearing","primary_cat":"astro-ph.HE","submitted_at":"2025-11-12T19:00:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"High-resolution GRMHD simulations show that tearing of tilted accretion disks around rapidly spinning supermassive black holes drives order-of-magnitude variability in continuum and broad-line luminosities on months-to-years timescales, explaining changing-look AGN.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2507.20232","ref_index":48,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A Systematic Search for Active Galactic Nucleus Flares in ZTF Data Release 23","primary_cat":"astro-ph.HE","submitted_at":"2025-07-27T11:30:53+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Systematic search of ZTF DR23 data yields catalogs of 28,504 coarse and 1,984 refined AGN flares with public release.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}